Search Results - "Muchovej, S J C"
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The C-Band All-Sky Survey (C-BASS): constraining diffuse Galactic radio emission in the North Celestial Pole region
Published in Monthly notices of the Royal Astronomical Society (11-05-2019)“…ABSTRACT The C-Band All-Sky Survey (C-BASS) is a high sensitivity all-sky radio survey at an angular resolution of 45 arcmin and a frequency of 4.7 GHz. We…”
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Using cm observations to constrain the abundance of very small dust grains in Galactic cold cores
Published in Monthly notices of the Royal Astronomical Society (01-03-2016)“…In this analysis, we illustrate how the relatively new emission mechanism, known as spinning dust, can be used to characterize dust grains in the interstellar…”
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3
The C-Band All-Sky Survey (C-BASS): design and implementation of the northern receiver
Published in Monthly notices of the Royal Astronomical Society (01-03-2014)“…The C-Band All-Sky Survey is a project to map the full sky in total intensity and linear polarization at 5 GHz. The northern component of the survey uses a…”
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4
CARMA observations of Galactic cold cores: searching for spinning dust emission
Published in Monthly notices of the Royal Astronomical Society (11-11-2015)“…We present the first search for spinning dust emission from a sample of 34 Galactic cold cores, performed using the CARMA interferometer. For each of our…”
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5
The C-Band All-Sky Survey (C-BASS): design and capabilities
Published in Monthly notices of the Royal Astronomical Society (01-11-2018)“…The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarization survey at a frequency of 5 GHz, designed to provide complementary data to the all-sky…”
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6
C-Band All-Sky Survey: a first look at the Galaxy
Published in Monthly notices of the Royal Astronomical Society (21-04-2015)“…We present an analysis of the diffuse emission at 5 GHz in the first quadrant of the Galactic plane using two months of preliminary intensity data taken with…”
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The C-Band All-Sky Survey (C-BASS): digital backend for the northern survey
Published in Monthly notices of the Royal Astronomical Society (21-04-2019)“…Abstract The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarization survey at a frequency of 5 GHz, designed to provide data complementary to the…”
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8
Astronomical receiver modelling using scattering matrices
Published in Monthly notices of the Royal Astronomical Society (11-01-2015)“…Proper modelling of astronomical receivers is vital: it describes the systematic errors in the raw data, guides the receiver design process, and assists data…”
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The C-Band All-Sky Survey (C-BASS): Digital backend for the northern survey
Published 29-01-2019“…MNRAS, 484, 5377-5388 (2019 April 21) The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarization survey at a frequency of 5 GHz, designed to provide…”
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10
The C-Band All-Sky Survey (C-BASS): Constraining diffuse Galactic radio emission in the North Celestial Pole region
Published 19-02-2019“…The C-Band All-Sky Survey C-BASS is a high-sensitivity all-sky radio survey at an angular resolution of 45 arcmin and a frequency of 4.7 GHz. We present a…”
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Journal Article -
11
The C-Band All-Sky Survey (C-BASS): Design and capabilities
Published 19-07-2018“…The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarisation survey at a frequency of 5 GHz, designed to provide complementary data to the all-sky…”
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12
THE CONTRIBUTION OF RADIO GALAXY CONTAMINATION TO MEASUREMENTS OF THE SUNYAEV-ZEL'DOVICH DECREMENT IN MASSIVE GALAXY CLUSTERS AT 140 GHz WITH BOLOCAM
Published in The Astrophysical journal (20-02-2013)“…We describe in detail our characterization of the compact radio source population in 140 GHz Bolocam observations of a set of 45 massive galaxy clusters. We…”
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13
Using cm Observations to Constrain the Abundance of Very Small Dust Grains in Galactic Cold Cores
Published 20-11-2015“…In this analysis we illustrate how the relatively new emission mechanism known as spinning dust can be used to characterize dust grains in the interstellar…”
Get full text
Journal Article -
14
CARMA Observations of Galactic Cold Cores: Searching for Spinning Dust Emission
Published 31-07-2015“…We present the first search for spinning dust emission from a sample of 34 Galactic cold cores, performed using the CARMA interferometer. For each of our cores…”
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15
A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10$^{15}$M$_{\odot}$ Galaxy Cluster at z=0.7
Published 03-11-2015“…We present an initial study of the mass and evolutionary state of a massive and distant cluster, RCS2 J232727.6-020437. This cluster, at z=0.6986, is the…”
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16
Astronomical Receiver Modelling Using Scattering Matrices
Published 20-10-2014“…Proper modelling of astronomical receivers is vital: it describes the systematic errors in the raw data, guides the receiver design process, and assists data…”
Get full text
Journal Article -
17
A multi-wavelength mass analysis of RCS2 J232727.6-020437, A ∼3 × 10{sup 15}M{sub ⊙} galaxy cluster at z = 0.7
Published in The Astrophysical journal (20-11-2015)“…We present an initial study of the mass and evolutionary state of a massive and distant cluster, RCS2 J232727.6-020437. This cluster, at z = 0.6986, is the…”
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A MULTI-WAVELENGTH MASS ANALYSIS OF RCS2 J232727.6-020437, A ∼3 × 1015 M GALAXY CLUSTER AT z = 0.7 Based on observations obtained with : MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii; the NASA/ESA Hubble Space Telescope (HST), o
Published in The Astrophysical journal (12-11-2015)“…ABSTRACT We present an initial study of the mass and evolutionary state of a massive and distant cluster, RCS2 J232727.6-020437. This cluster, at z = 0.6986,…”
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Journal Article -
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A MULTI-WAVELENGTH MASS ANALYSIS OF RCS2 J232727.6-020437, A ∼3 × 10 15 M ⊙ GALAXY CLUSTER AT z = 0.7
Published in The Astrophysical journal (12-11-2015)Get full text
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20
C-Band All-Sky Survey: A First Look at the Galaxy
Published 24-01-2015“…We present an analysis of the diffuse emission at 5 GHz in the first quadrant of the Galactic plane using two months of preliminary intensity data taken with…”
Get full text
Journal Article